Towards Axionic Starobinsky-like Inflation in String Theory

Understand

It is shown that Starobinsky-like potentials can be realized in non-geometric flux compactifications of string theory, where the inflaton involves an axion whose shift symmetry can protect UV-corrections to the scalar potential.

• For that purpose we evaluate the backreacted, uplifted F-term axion-monodromy potential, which interpolates between a quadratic and a Starobinsky-like form.
• Limitations due to the requirements of having a controlled approximation of the UV theory and of realizing single-field inflation are discussed.